Publié: 2013 Jun 22 1210 UTC
Eruptive (C-class flares expected, probability >=50%)
Quiet (A<20 and K<4)
Quiet
| Flux de 10 cm | Ap | |
|---|---|---|
| 22 Jun 2013 | 140 | 019 |
| 23 Jun 2013 | 145 | 005 |
| 24 Jun 2013 | 145 | 003 |
The background X-ray radiation is near the top of the B-level. NOAA AR 1777 has a probability of more than 50% to flare in the C-level. M-flares are still possible. Solar wind speed is around 600 km/s. The density and the magnetic field decreased. This behaviour of the solar wind parameters is a typical coronal hole signature: a co-rotating interaction region with relatively high density and compressed magnetic field is followed by the actual fast solar wind emanating from the coronal hole itself. This is a typical lower density plasma. Geomagnetic conditions returned to quiet/unsettled conditions.
Estimation du nombre international de taches solaires (ISN) pour aujourd'hui : 083, sur la base de 09 stations.
| Nombre de Wolf, observé par Catania | /// |
| Flux solaire à 10 cm | 133 |
| AK Chambon La Forêt | 027 |
| AK Wingst | 020 |
| Ap estimé | 022 |
| Nombre international de taches solaires estimé | 095 - Basé sur 17 stations |
| Jour | Commencer | Max | Fin | Loc | Force | OP | 10cm | Catania/NOAA | Types de sursaut radio | |
|---|---|---|---|---|---|---|---|---|---|---|
| Aucun | ||||||||||
Données fournies par le Solar Influences Data analysis Center© - SIDC - Traité par SpaceWeatherLive
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